, provisional designation , is a background asteroid and binary system from the inner regions of the asteroid belt. It was discovered on 11 October 1985, by astronomer by T. F. Fric and Richard Gilbrech at the Palomar Observatory in California. It is the only minor-planet discovery for these two astronomers. The stony L-type asteroid measures approximately in diameter and has a rotation period of 2.7 hours. Its 1.2-kilometer sized minor-planet moon was discovered in July 2007 and announced the following month. Orbit and classification is a non-family asteroid from the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. Based on osculating Keplerian orbital elements, the asteroid has also been classified as a member of the Flora family (), a giant asteroid family and the largest family of stony asteroids in the main-belt. It orbits the Sun in the inner asteroid belt at a distance of 1.7–2.6 AU once every 3 years and 2 months (1,164 days; semi-major axis of 2.17 AU). Its orbit has an eccentricity of 0.19 and an inclination of 4° with respect to the ecliptic. It was first observed as at the former Alma-Ata Observatory in September 1953. The body's observation arc begins with its observation as at Crimea–Nauchnij in December 1979, or almost 6 years prior to its official discovery observation at Palomar Observatory. Numbering and naming This minor planet was permanently numbered by the Minor Planet Center on 17 March 1995 (). As of 2018, it has not been named. Physical characteristics In the SDSS-based taxonomy, is an unusual L-type asteroid. Rotation period In June 2010, a rotational lightcurve of was obtained from photometric observations by Australian astronomers David Higgins and Julian Oey at the Hunters Hill and Leura Observatory . Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of 0.35 magnitude (). Several concurring period determinations in the range of 2.7091 to 2.710 hours with an amplitude of 0.26 to 0.36 magnitude were also made between 2007 and 2013 (). Satellite During a previous photometric observation by David Higgins on 15 July 2007, it was revealed that is a binary asteroid with a minor-planet moon in its orbit. The discovery was announced on 2 August 2007. The satellite, provisional designation S/2007 (6265) 1, measures approximately 1.16 kilometers. It is separated by 8 km from its primary, orbiting it once every 15